activity
20002022
most citedDeep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations

224 citations · 1.1k across the 31 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

10 papers · 1 filter

astro-ph.IM202116 cited

Dual Polarization Measurements of MWA Beampatterns at 137 MHz

A. Chokshi, J. L. B. Line, N. Barry +5

The wide adoption of low-frequency radio interferometers as a tool for deeper and higher resolution astronomical observations has revolutionised radio astronomy. Despite their cons…

astro-ph.IM2020

The Impact of Tandem Redundant/Sky-Based Calibration in MWA Phase II Data Analysis

Zheng Zhang, Jonathan C. Pober, Wenyang Li +26

Precise instrumental calibration is of crucial importance to 21-cm cosmology experiments. The Murchison Widefield Array's (MWA) Phase II compact configuration offers us opportuniti…

astro-ph.IM202022 cited

Modelling and peeling extended sources with shapelets: a Fornax A case study

J. L. B. Line, D. A. Mitchell, B. Pindor +6

To make a power spectrum (PS) detection of the 21 cm signal from the Epoch of Reionisation (EoR), one must avoid/subtract bright foreground sources. Sources such as Fornax A presen…

astro-ph.IM2018

Assessment of ionospheric activity tolerances for Epoch of Reionisation science with the Murchison Widefield Array

Cathryn M. Trott, C. H. Jordan, S. G. Murray +20

Structure imprinted in foreground extragalactic point sources by ionospheric refraction has the potential to contaminate Epoch of Reionisation (EoR) power spectra of the 21~cm emis…

astro-ph.IM2018

In situ measurement of MWA primary beam variation using ORBCOMM

J. L. B. Line, B. McKinley, J. Rasti +21

We provide the first in situ measurements of antenna element (tile) beam shapes of the Murchison Widefield Array (MWA), a low radio-frequency interferometer and an SKA precursor. M…

astro-ph.IM2018

Comparing Redundant and Sky Model Based Interferometric Calibration: A First Look with Phase II of the MWA

W. Li, J. C. Pober, B. J. Hazelton +53

Interferometric arrays seeking to measure the 21 cm signal from the Epoch of Reionization must contend with overwhelmingly bright emission from foreground sources. Accurate recover…